Data di Pubblicazione:
2010
Citazione:
Constraining the S-factor for 15N(p,gamma)16O reaction at astrophysical energies / P. J. Le Blanc, G. Imbriani, J. Gorres, M. Junker, R. Azuma, M. Beard, D. Bemmerer, A. Best, C. Broggini, A. Caciolli, P. Corvisiero, H. Costantini, M. Couder, R. DeBoer, Z. Elekes, S. Falahat, A. Formicola, Zs. Fulop, G. Gervino, A. Guglielmetti, C. Gustavino, Gy. Gyurky, F. Kappeler, A. Kontos, R. Kuntz, H. Leiste, A. Lemut, Q. Li, B. Limata, M. Marta, C. Mazzocchi, R. Menegazzo, S. O. Brien, A. Palumbo, P. Prati, V. Roca, C. Rolfs, C. Rossi Alvarez, E. Somorjai, E. Stech, O. Straniero, F. Strieder, W. Tan, F. Terrasi, H. P. Trautvetter, E. Uberseder, M. Wiescher. - In: PHYSICAL REVIEW. C, NUCLEAR PHYSICS. - ISSN 0556-2813. - 82:5(2010), pp. 055804.055804.1-055804.055804.10. [10.1103/PhysRevC.82.055804]
Abstract:
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the CNO cycles redistributing the carbon and nitrogen abundances into the oxygen range. The reaction is dominated by two broad resonances, at Ep=338 and 1028 keV, and a direct capture contribution to the ground state of 16O. Interference effects between these contributions both in the low-energy region (Ep<338 keV) and between the two resonances (338
Tipologia IRIS:
01 - Articolo su periodico
Elenco autori:
P.J. Le Blanc, G. Imbriani, J. Gorres, M. Junker, R. Azuma, M. Beard, D. Bemmerer, A. Best, C. Broggini, A. Caciolli, P. Corvisiero, H. Costantini, M. Couder, R. Deboer, Z. Elekes, S. Falahat, A. Formicola, Z.S. Fulop, G. Gervino, A. Guglielmetti, C. Gustavino, G.Y. Gyurky, F. Kappeler, A. Kontos, R. Kuntz, H. Leiste, A. Lemut, Q. Li, B. Limata, M. Marta, C. Mazzocchi, R. Menegazzo, S.O. Brien, A. Palumbo, P. Prati, V. Roca, C. Rolfs, C. Rossi Alvarez, E. Somorjai, E. Stech, O. Straniero, F. Strieder, W. Tan, F. Terrasi, H.P. Trautvetter, E. Uberseder, M. Wiescher
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